© Andy Roberts 1997. Pictured comet is C/1995 O1 Hale-Bopp.

Comet 73P/Schwassmann-Wachmann passes perihelion

Dominic Ford, Editor
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Comet 73P/Schwassmann-Wachmann will make its closest approach to the Sun on 16 August, at a distance of 0.91 AU.

From Cambridge on the day of perihelion it will not be observable – it will reach its highest point in the sky during daytime and will be no higher than 5° above the horizon at dusk.

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The events that comprise the 2006 apparition of 73P/Schwassmann-Wachmann are as follows:

Date Event
16 Aug 2006Comet 73P/Schwassmann-Wachmann passes perihelion

The table below lists the times when 73P/Schwassmann-Wachmann will be visible from Cambridge day-by-day through its apparition:

Date Constellation Comet visibility
26 Jul 2006VirgoNot observable
28 Jul 2006VirgoNot observable
30 Jul 2006VirgoNot observable
01 Aug 2006VirgoNot observable
03 Aug 2006VirgoNot observable
05 Aug 2006VirgoNot observable
07 Aug 2006VirgoNot observable
09 Aug 2006VirgoNot observable
11 Aug 2006VirgoNot observable
13 Aug 2006VirgoNot observable
15 Aug 2006VirgoNot observable
17 Aug 2006VirgoNot observable
19 Aug 2006VirgoNot observable
21 Aug 2006VirgoNot observable
23 Aug 2006VirgoNot observable
25 Aug 2006VirgoNot observable
27 Aug 2006VirgoNot observable
29 Aug 2006VirgoNot observable
31 Aug 2006VirgoNot observable
02 Sep 2006HydraNot observable
04 Sep 2006LibraNot observable

A more detailed table of 73P/Schwassmann-Wachmann's position on each night is available here. A diagram of the orbit of 73P/Schwassmann-Wachmann is available here.

Finder chart

The chart below shows the path of 73P/Schwassmann-Wachmann over the course of its apparition, as calculated from the orbital elements published by the Minor Planet Center (MPC). It is available for download, either on dark background, in PNG, PDF or SVG formats, or on a light background, in PNG, PDF or SVG formats. It was produced using StarCharter.

Comet brightnesses

Comets are intrinsically highly unpredictable objects, since their brightness depends on the scattering of sunlight from dust particles in the comet's coma and tail. This dust is continually streaming away from the comet's nucleus, and its density at any particular time is governed by the rate of sublimation of the ice in the comet's nucleus, as it is heated by the Sun's rays. It also depends on the amount of dust that is mixed in with that ice. This is very difficult to predict in advance, and can be highly variable even between successive apparitions of the same comet.

In consequence, while the future positions of comets are usually known with a high degree of confidence, their future brightnesses are not. For most comets, we do not publish any magnitude estimates at all. For the few comets where we do make estimates, we generally prefer the BAA's magnitude parameters to those published by the Minor Planet Center, since they are typically updated more often.

No estimate for the brightness of comet 73P/Schwassmann-Wachmann is currently available.

The comet's position at perihelion will be:

Object Right Ascension Declination Constellation Magnitude
Comet 73P/Schwassmann-Wachmann 13h07m30s 11°12'S Virgo 9.9

The coordinates are given in J2000.0.

The sky on 11 Dec 2024

The sky on 11 December 2024
Sunrise
07:01
Sunset
16:11
Twilight ends
17:52
Twilight begins
05:19

10-day old moon
Waxing Gibbous

89%

10 days old

Planets
Rise Culm. Set
Mercury 05:55 10:46 15:36
Venus 10:11 14:51 19:31
Moon 13:25 20:28 03:45
Mars 19:28 02:57 10:26
Jupiter 15:45 23:15 06:45
Saturn 11:48 17:20 22:51
All times shown in EST.

Source

This event was automatically generated on the basis of orbital elements published by the Minor Planet Center (MPC) , and is updated whenever new elements become available. It was last updated on 11 Dec 2024.

Image credit

© Andy Roberts 1997. Pictured comet is C/1995 O1 Hale-Bopp.

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Cambridge

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42.38°N
71.11°W
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